The best astronomical site on earth? A modern optical/infrared telescope is only as good as its site. We have previously shown that the infrared skies above the South Pole are up to 100 times darker than skies elsewhere, leading to enormous potential gains in sensitivity. We now seek to extend these measurements to Antarctic sites that are even higher, drier and colder than the South Pole. These are expected to be the best observing sites on Earth, paving the way for the deployment of telescop ....The best astronomical site on earth? A modern optical/infrared telescope is only as good as its site. We have previously shown that the infrared skies above the South Pole are up to 100 times darker than skies elsewhere, leading to enormous potential gains in sensitivity. We now seek to extend these measurements to Antarctic sites that are even higher, drier and colder than the South Pole. These are expected to be the best observing sites on Earth, paving the way for the deployment of telescopes of unprecedented sensitivity able to explore the origins of planets, stars and galaxies.
Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989069
Funder
Australian Research Council
Funding Amount
$450,000.00
Summary
A New Digital Radar for Studies in Solar-Terrestrial and Atmospheric Physics. Australia is a world leader in the development of High Frequency (HF) radar surveillance systems, such as JORN (Jindalee over-the-horizon radar). However, Australia's ability to support these operations and remain a leader in these fields depends on its capacity to nurture expertise and train new personnel in these areas. The new HF radar system will play a crucial role in this respect, providing (i) high-level trainin ....A New Digital Radar for Studies in Solar-Terrestrial and Atmospheric Physics. Australia is a world leader in the development of High Frequency (HF) radar surveillance systems, such as JORN (Jindalee over-the-horizon radar). However, Australia's ability to support these operations and remain a leader in these fields depends on its capacity to nurture expertise and train new personnel in these areas. The new HF radar system will play a crucial role in this respect, providing (i) high-level training in radar technology and associated science, (ii) a test bed for the development of new instrumental and data analysis techniques, (c) new information on the source of ionospheric perturbations that can affect the performance of JORN, and (d) data important for Australia's space weather prediction community, via IPS (Ionospheric Prediction Service) Radio and Space Services.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0560872
Funder
Australian Research Council
Funding Amount
$142,138.00
Summary
The Buckland Park Lidar Facility. This project will develop a laser radar (lidar) facility to operate as a test bed for studies in atmospheric physics, space physics, optics and astronomy.
A large aperture Sodium lidar for investigating the middle atmosphere (10-100 km). We will create a world-leading sodium lidar for remote sensing of the mesosphere and lower thermosphere (MLT) regions of the atmosphere, by developing a novel solid-state sodium light source and using the Cangaroo-1 telescope. It will provide the most accurate measurements ever of the temperature profile and wind velocities in the MLT for much needed input into models of the atmosphere. The addition of this capabi ....A large aperture Sodium lidar for investigating the middle atmosphere (10-100 km). We will create a world-leading sodium lidar for remote sensing of the mesosphere and lower thermosphere (MLT) regions of the atmosphere, by developing a novel solid-state sodium light source and using the Cangaroo-1 telescope. It will provide the most accurate measurements ever of the temperature profile and wind velocities in the MLT for much needed input into models of the atmosphere. The addition of this capability to the suite of atmospheric monitoring instruments at the Buckland Park field station will create a major international research facility, unrivalled in the world.Read moreRead less
Polar Cap Region Boundary Dynamics. Geomagnetic storms have the potential to severely impair critical technology infrastructure. Consequences of strong geomagnetic activity can include power failures, pipeline corrosion, satellite failures, inaccurate GPS positioning and radio navigation. Knowledge of how, where and under which conditions this activity occurs is therefore crucial. The primary aim of this project is to extend our knowledge of the mechanisms by which this activity occurs. This wor ....Polar Cap Region Boundary Dynamics. Geomagnetic storms have the potential to severely impair critical technology infrastructure. Consequences of strong geomagnetic activity can include power failures, pipeline corrosion, satellite failures, inaccurate GPS positioning and radio navigation. Knowledge of how, where and under which conditions this activity occurs is therefore crucial. The primary aim of this project is to extend our knowledge of the mechanisms by which this activity occurs. This work will consolidate Australia's international space profile and provide excellent training in this field, helping Australia's future technology development.Read moreRead less
Ground based monitoring of plasma dynamics in the magnetosphere. We will use a new technique to study the plasmapause, a fundamental and highly dynamic boundary in geospace. This is usually examined using spacecraft and ground-based VLF measurements, but these suffer several limitations. We have developed the ability to monitor plasma density in geospace, by measuring the resonant frequency of geomagnetic field line oscillations. This project will use data from extensive ground magnetometer a ....Ground based monitoring of plasma dynamics in the magnetosphere. We will use a new technique to study the plasmapause, a fundamental and highly dynamic boundary in geospace. This is usually examined using spacecraft and ground-based VLF measurements, but these suffer several limitations. We have developed the ability to monitor plasma density in geospace, by measuring the resonant frequency of geomagnetic field line oscillations. This project will use data from extensive ground magnetometer arrays to thus study the spatial and temporal variation in particle density near the plasmapause. Comparison with VLF and spacecraft measurements will provide new information on the plasma composition and dynamics in this important region.Read moreRead less
Monitoring and Predicting Near Real Time Ionospheric Activities with Multi-satellite Data. The ionosphere affects the transmission of electromagnetic waves, which can result in disturbance or intermission of radio signals being used for communication, navigation and other microwave systems. This project aims to monitor and predict near real-time ionospheric activities with multi-satellite data. The expected outcomes include: 1) an innovative algorithm to calculate the Total Electron Content from ....Monitoring and Predicting Near Real Time Ionospheric Activities with Multi-satellite Data. The ionosphere affects the transmission of electromagnetic waves, which can result in disturbance or intermission of radio signals being used for communication, navigation and other microwave systems. This project aims to monitor and predict near real-time ionospheric activities with multi-satellite data. The expected outcomes include: 1) an innovative algorithm to calculate the Total Electron Content from multi-satellite data; 2) an automated software package for mapping 3-dimensional ionospheric profile; and 3) an improved understanding of the detailed processes and causes of ionospheric events, that can enhance the space weather services for Australia and the world.Read moreRead less
Molecular signatures of complex photodissociation reactions. All energy on earth comes from the sun, either directly (e.g photosynthesis) or indirectly (e.g fossil fuels). Photochemistry is the study of how this light is absorbed and what happens to a molecule afterwards. Despite significant experimental and theoretical advances in the past decade (some in our lab), scientists still cannot predict the outcomes of most photochemical reactions. In this project we will determine the reactivity o ....Molecular signatures of complex photodissociation reactions. All energy on earth comes from the sun, either directly (e.g photosynthesis) or indirectly (e.g fossil fuels). Photochemistry is the study of how this light is absorbed and what happens to a molecule afterwards. Despite significant experimental and theoretical advances in the past decade (some in our lab), scientists still cannot predict the outcomes of most photochemical reactions. In this project we will determine the reactivity of several small, fundamental organic molecules. Not only are these molecules pollutants around our cities, but discovery of how they react in the presence of light will allow us to understand and predict the photochemistry of a much wider range of organic species.Read moreRead less
Coherent LIDAR for Monitoring Air Pollution and Atmospheric Wind-fields. Industry, government and civil defence urgently require compact, field deployable sensors that can measure winds and monitor pollution in the atmospheric boundary layer. Without these sensors they are unable to measure and make informed decisions about windborne dispersion of industrial emissions, environmental pollutants, and chemical/biological toxins under operational conditions. The project will develop eye-safe cohere ....Coherent LIDAR for Monitoring Air Pollution and Atmospheric Wind-fields. Industry, government and civil defence urgently require compact, field deployable sensors that can measure winds and monitor pollution in the atmospheric boundary layer. Without these sensors they are unable to measure and make informed decisions about windborne dispersion of industrial emissions, environmental pollutants, and chemical/biological toxins under operational conditions. The project will develop eye-safe coherent lidar (light detection and ranging) systems that can measure wind velocities at ranges of up to 10 km with an accuracy of about 1 m/s, and can be deployed to field sites as required. The technology will be of major interest to the commercial sector.Read moreRead less
Vibrational Spectroscopy and Imaging from Interstellar Dust to Life. The outcome of this project will result in a more thorough understanding of the role of water in the atmosphere and in the Greenhouse effect, and will provide information leading to more accurate modelling of Global warming. The results will also lead to new insights into interstellar chemistry, the chemistry of cometary dust and the origins of life.